activity
20242026
collaborators

6 papers

astro-ph.HE2026

The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654

Dev R. Sadaula, Sibasish Laha, Eileen T. Meyer +27

We present results from a comprehensive multi-wavelength monitoring campaign of the changing-look active galactic nucleus 1ES 1927+654 during the onset and evolution of a relativis…

astro-ph.HE2026

Blueshifted lines from the inner accretion disc's rotation can explain quasar absorption "forests''

Amelia M. Hankla, Fergus J. E. Baker, Daniel R. Wilkins +1

Recent XRISM observations of active galactic nuclei such as PDS 456 have revealed ``forests'' of absorption lines best modeled by five distinct absorption zones with varying large…

astro-ph.HE2025

An outflow from the X-ray corona as the origin of millimeter emission from radio-quiet AGN

A. Hankla, A. Philippov, R. Mbarek +4

Recent observations of radio-quiet active galactic nuclei (RQAGN) have shown the presence of millimeter emission, whose origin remains unknown, from within parsec scales of the cen…

astro-ph.HE2025

The inner structure and thermodynamics of a thin accretion disc

A. Hankla, J. Dexter, N. Scepi

Using three-dimensional general relativistic magnetohydrodynamic simulations with electron and proton thermodynamics and an electron cooling function, we probe the inner radial and…

astro-ph.HE2025

Multi-wavelength observations of a jet launch in real time from the post-changing-look Active Galaxy 1ES 1927+654

Sibasish Laha, Eileen T. Meyer, Dev R. Sadaula +34

We present results from a high cadence multi-wavelength observational campaign of the enigmatic changing look AGN 1ES 1927+654 from May 2022- April 2024, coincident with an unprece…

astro-ph.HE2024

X-ray properties of coronal emission in radio quiet Active Galactic Nuclei

Sibasish Laha, Claudio Ricci, John C. Mather +5

Active galactic nuclei (AGN) are powerful sources of panchromatic radiation. All AGN emit in X-rays, contributing around of the AGN bolometric luminosity. The X-ray e…